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<ri:Resource created="2012-08-22T12:08:46Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Intermediate-mass star-forming regions</title><shortName>J/AJ/140/462</shortName><identifier>ivo://CDS.VizieR/J/AJ/140/462</identifier><altIdentifier>doi:10.26093/cds/vizier.51400462</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Arvidsson K.</name></creator><creator><name>Kerton C.R.</name></creator><creator><name>Alexander M.J.</name></creator><creator><name>Kobulnicky H.A.</name></creator><creator><name>Uzpen B.</name></creator><date role="Updated">2017-06-19T07:58:15Z</date><date role="Created">2012-08-22T12:08:46Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>stellar-associations</subject><subject>h-ii-regions</subject><subject>infrared-sources</subject><subject>galaxy-planes</subject><subject>milky-way-galaxy</subject><description>In an effort to understand the factors that govern the transition from low- to high-mass star formation, for the first time we identify a sample of intermediate-mass star-forming regions (IM SFRs) where stars up to (but not exceeding) ~8M_{sun}_ are being produced. We use IRAS colors and Spitzer Space Telescope mid-IR images, in conjunction with millimeter continuum and ^13^CO maps, to compile a sample of 50 IM SFRs in the inner Galaxy. These are likely to be precursors to Herbig AeBe stars and their associated clusters of low-mass stars.</description><source format="bibcode">2010AJ....140..462A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/140/462</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/1153">J/ApJ/699/1153 : Kinematic dist. to GRS molecular clouds (Roman-Duval+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/182/131">J/ApJS/182/131 : Molecular clouds and clumps in the GRS (Rathborne+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/188/123">J/ApJS/188/123 : The Bolocam Galactic Plane Survey. 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Associated CO velocity from the GRS (Jackson et al., 2006ApJS..163..145J)</description><unit>km/s</unit><ucd>phys.veloc;pos.lsr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dV</name><description>? Width of the associated CO feature {Delta}V</description><unit>km/s</unit><ucd>meta.id.assoc;pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dnear</name><description>? Near distance</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>dfar</name><description>? Far distance</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Dist</name><description>? Adopted distance used in subsequent analysis</description><unit>kpc</unit><ucd>pos.distance;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Flag</name><description>Flag (G1)</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Diam</name><description>? Diameter, calculated using the adopted distance</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Diam2</name><description>? Second diameter, calculated using the adopted distance</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>LIR</name><description>? Infrared luminosity (taken from table4)</description><unit>ksolLum</unit><ucd>phys.luminosity;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>LIR2</name><description>? Second infrared luminosity (taken from table4)</description><unit>ksolLum</unit><ucd>phys.luminosity;em.IR</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MLTE</name><description>? LTE mass (taken from table5)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>MLTE2</name><description>? Second LTE mass (taken from table5)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Ap</name><description>Aperture radius</description><unit>arcsec</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>F3.6</name><description>Spitzer/IRAC 3.6um flux density</description><unit>Jy</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F3.6</name><description>1{sigma} total uncertainty on F3.6</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F4.5</name><description>Spitzer/IRAC 4.5um flux density</description><unit>Jy</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F4.5</name><description>1{sigma} total uncertainty on F4.5</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F5.8</name><description>Spitzer/IRAC 5.8um flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F5.8</name><description>1{sigma} total uncertainty on F5.8</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F8.0</name><description>Spitzer/IRAC 8.0um flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F8.0</name><description>1{sigma} total uncertainty on F8.0</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F24</name><description>Spitzer/MIPS 24um flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_F24</name><description>1{sigma} total uncertainty on F24</description><unit>Jy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F60</name><description>IRAS PSC 60um flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.30-60um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F100</name><description>IRAS PSC 100um flux density</description><unit>Jy</unit><ucd>phot.flux.density;em.IR.60-100um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Lnear</name><description>? 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